Zeta Ophiuchi

Zeta Ophiuchi
Observation data
Epoch J2000      Equinox J2000
Constellation Ophiuchus
Right ascension 16h 37m 09.5s
Declination -10° 34′ 01.4″
Apparent magnitude (V) 2.54

This infrared image from NASA's WISE telescope shows the runaway star Zeta Ophiuchi as it creates a bright shockwave (yellow arc) in an interstellar dust cloud as it zooms through space.
Characteristics
Spectral type O9 III
U−B color index -0.86
B−V color index 0.02
Variable type Gamma Cass.
Astrometry
Radial velocity (Rv) -15 km/s
Proper motion (μ) RA: 13.07 mas/yr
Dec.: 25.44 mas/yr
Parallax (π) 7.12 ± 0.71 mas
Distance 458 ly
(140 pc)
Absolute magnitude (MV) -3.20
Details
Mass 20 M
Radius 8 R
Luminosity 68,000 L
Temperature 33,500 K
Metallicity titanium
Rotation 380 km/s.
Age 4 × 106 years
Other designations
13 Oph, HR 6175, BD -10°4350, HD 149757, SAO 160006, FK5 622, HIP 81377.

Zeta Ophiuchi (ζ Oph, ζ Ophiuchi) is a star located in the constellation of Ophiuchus. It was a member of indigenous Arabic asterism al-Nasaq al-Yamānī, "the Southern Line" of al-Nasaqān "the Two Lines".,[1] along with α Ser (Unukalhai), δ Ser (Qin, Tsin), ε Ser (Ba, Pa), δ Oph (Yed Prior), ε Ser (Yed Posterior) and γ Oph (Tsung Ching).[2]

According to the catalogue of stars in the Technical Memorandum 33-507 - A Reduced Star Catalog Containing 537 Named Stars, al-Nasaq al-Yamānī or Nasak Yamani were the title for two stars :δ Ser as Nasak Yamani I and ε Ser as Nasak Yamani II (exclude this star, α Ser, δ Oph, ε Oph and γ Oph)[3]

In Chinese, 天市右垣 (Tiān Shì Yòu Yuán), meaning Right Wall of Heavenly Market Enclosure, refers to an asterism which is represent eleven old states in China which is marking the right borderline of the enclosure, consisting of ζ Ophiuchi, β Herculis, γ Herculis, κ Herculis, γ Serpentis, β Serpentis, α Serpentis, δ Serpentis, ε Serpentis, δ Ophiuchi and ε Ophiuchi.[4] Consequently, ζ Ophiuchi itself is known as 天市右垣十一 (Tiān Shì Yòu Yuán shíyī, English: the Eleventh Star of Right Wall of Heavenly Market Enclosure), represent the state Han (韓),[5][6][7] together with 35 Capricorni in Twelve States (asterism).

Properties

Although ζ Ophiuchi is a hot blue supergiant star it appears reddish due to interstellar dust that absorbs much of blue light. In fact, were it not for this dust, ζ Ophiuchi would shine several times brighter and be among the very brightest visible. ζ Ophiuchi is roughly half way through the initial phase of its stellar evolution and will within the next few million years expand into a supergiant star before ending its life in a spectacular supernova.[8][9]

Discoveries announced in early 2011 show that ζ Ophiuchi is moving through space at 87,000 km/h (54,000 mph), having likely been ejected from orbit around a more massive star that was destroyed in its own supernova blast. Due to this high proper motion in combination with high intrinsic brightness and its current location in a dust-rich area of the galaxy, the star is creating a bow-shock in the direction of motion. This shock has been made visible via NASA's Wide-field Infrared Survey Explorer.[10]

References

  1. ^ Kunitzsch, P., Smart, T., (2006). A Dictionary of Modern Star names: A Short Guide to 254 Star names and Their Derivations (Second Revised ed.). Cambridge, MA: Sky Publishing. p. 31. ISBN 1931559449. 
  2. ^ Allen, R. H. (1963). Star Names: Their Lore and Meaning (Reprint ed.). New York, NY: Dover Publications Inc. p. 243. ISBN 0486210790. http://penelope.uchicago.edu/Thayer/E/Gazetteer/Topics/astronomy/_Texts/secondary/ALLSTA/Hercules*.html. Retrieved 2010-12-12. 
  3. ^ Jack W. Rhoads - Technical Memorandum 33-507-A Reduced Star Catalog Containing 537 Named Stars, Jet Propulsion Laboratory, California Institute of Technology; November 15, 1971
  4. ^ (Chinese) 中國星座神話, written by 陳久金. Published by 台灣書房出版有限公司, 2005, ISBN 9789867332257.
  5. ^ Star Names - R.H.Allen p.302
  6. ^ (Chinese) 香港太空館 - 研究資源 - 亮星中英對照表, Hong Kong Space Museum. Accessed on line November 23, 2010.
  7. ^ (Chinese) English-Chinese Glossary of Chinese Star Regions, Asterisms and Star Name, Hong Kong Space Museum. Accessed on line November 23, 2010.
  8. ^ "HD 149757 -- Be Star". SIMBAD Astronomical Database. http://simbad.u-strasbg.fr/sim-id.pl?protocol=html&Ident=zeta+ophiuchi&NbIdent=1&Radius=10&Radius.unit=arcmin&CooFrame=FK5&CooEpoch=2000&CooEqui=2000&output.max=all&o.catall=on&output.mesdisp=N&Bibyear1=1983&Bibyear2=2005&Frame1=FK5&Frame2=FK4&Frame3=G&Equi1=2000.0&Equi2=1950.0&Equi3=2000.0&Epoch1=2000.0&Epoch2=1950.0&Epoch3=2000.0. Retrieved 2007-03-29. 
  9. ^ Zeta Oph
  10. ^ "Runaway Star Plows Through Space". http://www.jpl.nasa.gov/wise/newsfeatures.cfm?release=2011-026. Retrieved 2011-01-24.